Fixing NOTE in roman.rst

BradleySappington · Nov 27, 2024 · 948d3f2 · 948d3f2
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diff --git a/README.rst b/README.rst
@@ -28,9 +28,10 @@ imaging, coronagraphic, and spectroscopic modes.
 
 WebbPSF also supports simulating PSFs for the upcoming Nancy Grace Roman Space Telescope (formerly WFIRST),
 including its Wide Field Instrument and a preliminary version of the Coronagraph Instrument.
+
 .. note::
-The current Roman WFI optical model was provided by Goddard Space
-Flight Center circa 2021 (the Cycle 9 reference data); a new optical model is currently being implemented in WebbPSF.
+
+   The current Roman WFI optical model was provided by Goddard Space Flight Center circa 2021 (the Cycle 9 reference data); a new optical model is currently being implemented in WebbPSF.
 
 Developed by Marshall Perrin, Joseph Long, Shannon Osborne, Robel Geda, Bradley Sappington, Marcio Meléndez, 
 Charles-Philippe Lajoie, Jarron Leisenring, Neil Zimmerman, Keira Brooks, 

diff --git a/docs/roman.rst b/docs/roman.rst
@@ -24,8 +24,7 @@ The WFI model is based on the `Cycle 9 instrument reference information <https:/
 
 .. note::
 
-   The current Roman WFI optical model was provided by Goddard Space
-Flight Center circa 2021 (the Cycle 9 reference data); a new optical model is currently being implemented in WebbPSF.
+   The current Roman WFI optical model was provided by Goddard Space Flight Center circa 2021 (the Cycle 9 reference data); a new optical model is currently being implemented in WebbPSF.
 
 
 To work with the WFI model, import and instantiate it just like any of the JWST instruments::